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- W3000656572 abstract "Currently, most photometric studies of galaxies have only been done by treating a galaxy as a single point object or modeling them with a few axisymmetric components. The advent of IFU surveys has revolutionized the way we study galaxies. Despite its powerful capabilities, wide-area IFU surveys are only limited to local galaxies. The latest development in the spectral energy distribution (SED) fitting method makes it possible to implement the method on a pixel-to-pixel basis. piXedfit, pixelized SED fitting, is a python package that provides tools for obtaining spatially resolved stellar population properties of galaxies from multi-band imaging data. This package will be an essential tool for studying the stellar population properties of galaxies across a wide redshift range in the era of big data in photometry (from JWST, WFIRST, LSST, and Euclid)." @default.
- W3000656572 created "2020-01-23" @default.
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- W3000656572 date "2019-11-01" @default.
- W3000656572 modified "2023-09-23" @default.
- W3000656572 title "Spatially resolving properties of galaxies across cosmic time with piXedfit" @default.
- W3000656572 doi "https://doi.org/10.5281/zenodo.3554932" @default.
- W3000656572 hasPublicationYear "2019" @default.
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